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<front>
<journal-meta>
<journal-id>1409-2433</journal-id>
<journal-title><![CDATA[Revista de Matemática Teoría y Aplicaciones]]></journal-title>
<abbrev-journal-title><![CDATA[Rev. Mat]]></abbrev-journal-title>
<issn>1409-2433</issn>
<publisher>
<publisher-name><![CDATA[Centro de Investigaciones en Matemática Pura y Aplicada (CIMPA) y Escuela de Matemática, San José, Costa Rica.]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S1409-24332014000200002</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Lensing properties of the einasto profile in terms of the meijer G function]]></article-title>
<article-title xml:lang="es"><![CDATA[Propiedades del efecto lente para el perfil de einasto en términos de la función G de meijer]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Retana-Montenegro]]></surname>
<given-names><![CDATA[Edwin]]></given-names>
</name>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Frutos-Alfaro]]></surname>
<given-names><![CDATA[Francisco]]></given-names>
</name>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Universidad de Costa Rica Escuela de Física ]]></institution>
<addr-line><![CDATA[San Pedro ]]></addr-line>
<country>Costa Rica</country>
</aff>
<aff id="A02">
<institution><![CDATA[,Universidad de Costa Rica Escuela de Física ]]></institution>
<addr-line><![CDATA[San Pedro ]]></addr-line>
<country>Costa Rica</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>12</month>
<year>2014</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>12</month>
<year>2014</year>
</pub-date>
<volume>21</volume>
<numero>2</numero>
<fpage>189</fpage>
<lpage>198</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.sa.cr/scielo.php?script=sci_arttext&amp;pid=S1409-24332014000200002&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.sa.cr/scielo.php?script=sci_abstract&amp;pid=S1409-24332014000200002&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.sa.cr/scielo.php?script=sci_pdf&amp;pid=S1409-24332014000200002&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="es"><p><![CDATA[In N-body simulations of cold dark matter, it has been found that three-parameter models, particularly the Einasto profile, yield better fits to a wide range of dark matter haloes than two parameter models like the Navarro-Frenk-White profile. Recently, the analytical properties of the Einasto profile has been studied, allowing closed expressions for its surface mass density and lensing properties in terms of the Fox H and Meijer G functions, using a Mellin transform formalism. These expressions are valid for all values of the Einasto index in terms of the Fox H function, and valid for integer and half-integer values of Einasto index in terms of the Meijer G function. In this paper, we derive expressions for lensing properties of the Einasto profile for all rational values of the Einasto index in terms of theMeijer G function. Equivalency between these expressions and other recent results is also discussed]]></p></abstract>
<abstract abstract-type="short" xml:lang="en"><p><![CDATA[En simulaciones de N-cuerpos de materia oscura fría, se ha encontrado que modelos de tres parámetros, particularmente el perfil de Einasto, ofrece mejores ajustes para un amplio rango de halos de materia oscura que los modelos de dos parámetros como el perfil Navarro-Frenk-White. Recientemente, las propiedades analíticas del perfil de Einasto han sido estudiadas, lográdose expresiones cerradas para su densidad de masa superficial y propiedades de lente gravitational en términos de la función H de Fox, usando el formalismo de la transformada de Mellin. Estas expresiones son válidas para todos los valores del índice de Einasto en términos de la función H de Fox, y válidos para valores enteros y semi-enteros del índice de Einasto en términos de la función G de Meijer. En este artículo, se determinan expresiones para las propiedades de lente gravitational del perfil de Einasto para todos los valores racionales del índice de Einasto en términos de la función G de Meijer. La equivalencia entre estas expresiones y otros resultados recientes también es discutida.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[cosmology]]></kwd>
<kwd lng="en"><![CDATA[dark matter]]></kwd>
<kwd lng="en"><![CDATA[Meijer G function]]></kwd>
<kwd lng="es"><![CDATA[cosmología]]></kwd>
<kwd lng="es"><![CDATA[materia oscura]]></kwd>
<kwd lng="es"><![CDATA[función G de Meijer]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <div style="text-align: justify;">     <div style="text-align: center;"><font  style="font-family: Verdana; font-weight: bold;" size="4">Lensing properties of the einasto profile in terms of the meijer G function</font>    <br> </div> <font style="font-family: Verdana;" size="2"></font>    <br>     <div style="text-align: center;"><font  style="font-family: Verdana; font-weight: bold;" size="4">Propiedades del efecto lente para el perfil de einasto en t&eacute;rminos de la funci&oacute;n G de meijer</font>    <br> </div>     <br>     <div style="text-align: center;"><font style="font-family: Verdana;"  size="2">Edwin Retana-Montenegro<sup><a href="#1">*</a><a name="3"></a>+</sup> Francisco Frutos-Alfaro<sup><a href="#2">&#8224;</a><a name="4"></a>*</sup></font>    <br> </div>     <br> <hr style="width: 100%; height: 2px;">    ]]></body>
<body><![CDATA[<br> <font style="font-family: Verdana; font-weight: bold;" size="3">Abstract</font>    <br>     <br> <font style="font-family: Verdana;" size="2">In <span  style="font-style: italic;">N</span>-body simulations of cold dark matter, it has been found that three-parameter models, particularly the Einasto profile, yield better fits to a wide range of dark matter haloes than two parameter models like the Navarro-Frenk-White profile. Recently, the analytical properties of the Einasto profile has been studied, allowing closed expressions for its surface mass density and lensing properties in terms of the Fox <span style="font-style: italic;">H</span> and Meijer <span style="font-style: italic;">G</span> functions, using a Mellin transform formalism. These expressions are valid for all values of the Einasto index in terms of the Fox <span style="font-style: italic;">H</span> function, and valid for integer and half-integer values of Einasto index in terms of the Meijer <span  style="font-style: italic;">G</span> function. In this paper, we derive expressions for lensing properties of the Einasto profile for all rational values of the Einasto index in terms of theMeijer <span style="font-style: italic;">G</span> function. Equivalency between these expressions and other recent results is also discussed </font>    <br> <font style="font-family: Verdana;" size="2"></font>    <br> <font style="font-family: Verdana;" size="2"><span  style="font-weight: bold;">Keywords:</span> cosmology; dark matter; Meijer <span style="font-style: italic;">G</span> function.</font>    <br> <font style="font-family: Verdana;" size="2"></font>    <br> <font style="font-family: Verdana; font-weight: bold;" size="3">Resumen</font>    <br> <font style="font-family: Verdana;" size="2"></font>    <br> <font style="font-family: Verdana;" size="2">En simulaciones de <span  style="font-style: italic;">N</span>-cuerpos de materia oscura fr&iacute;a, se ha encontrado que modelos de tres par&aacute;metros, particularmente el perfil de Einasto, ofrece mejores ajustes para un amplio rango de halos de materia oscura que los modelos de dos par&aacute;metros como el perfil Navarro-Frenk-White. Recientemente, las propiedades anal&iacute;ticas del perfil de Einasto han sido estudiadas, logr&aacute;dose expresiones cerradas para su densidad de masa superficial y propiedades de lente gravitational en t&eacute;rminos de la funci&oacute;n <span style="font-style: italic;">H</span> de Fox, usando el formalismo de la transformada de Mellin. Estas expresiones son v&aacute;lidas para todos los valores del &iacute;ndice de Einasto en t&eacute;rminos de la funci&oacute;n <span  style="font-style: italic;">H</span> de Fox, y v&aacute;lidos para valores enteros y semi-enteros del &iacute;ndice de Einasto en t&eacute;rminos de la funci&oacute;n <span style="font-style: italic;">G</span> de Meijer. En este art&iacute;culo, se determinan expresiones para las propiedades de lente gravitational del perfil de Einasto para todos los valores racionales del &iacute;ndice de Einasto en t&eacute;rminos de la funci&oacute;n <span style="font-style: italic;">G</span> de Meijer. La equivalencia entre estas expresiones y otros resultados recientes tambi&eacute;n es discutida. </font>    <br> <font style="font-family: Verdana;" size="2"></font>    ]]></body>
<body><![CDATA[<br> <font style="font-family: Verdana;" size="2"><span  style="font-weight: bold;">Palabras clave:</span> cosmolog&iacute;a; materia oscura; funci&oacute;n <span style="font-style: italic;">G</span> de Meijer.</font>    <br> <font style="font-family: Verdana;" size="2"></font>    <br> <font style="font-family: Verdana;" size="2"><span  style="font-weight: bold;">Mathematics Subject Classification:</span> 33C60; 33E20.</font>    <br>     <br> <hr style="width: 100%; height: 2px;">    <br> <font style="font-family: Verdana;" size="2">Ver contenido disponible en pdf</font>    <br>     <br> <hr style="width: 100%; height: 2px;">    <br> <font style="font-family: Verdana; font-weight: bold;" size="3">References</font>    <br>     ]]></body>
<body><![CDATA[<br>     <!-- ref --><div style="text-align: left;"><font style="font-family: Verdana;"  size="2">[1] Adamchick, V. (1996) &#8220;Definite integration in Mathematica V3.0&#8221;, <span style="font-style: italic;">Mathematica in Education and Research</span>, <span style="font-weight: bold;">5</span>: 16&#8211;22.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958856&pid=S1409-2433201400020000200001&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[2] Baes, M.; Gentile, G. (2011) &#8220;Analytical expressions for the deprojected S&eacute;rsic model&#8221;, <span style="font-style: italic;">A &amp; A</span>, <span style="font-weight: bold;">525</span>: A136+ (1&#8211;7), <span style="font-style: italic;">arXiv:1009.4713</span>.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958859&pid=S1409-2433201400020000200002&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[3] Baes, M.; van Hese, E. (2011) &#8220;Analytical expressions for the deprojected S&eacute;rsic model. II. General expressions in terms of the Fox H function&#8221;, A <span style="font-style: italic;">&amp; A</span> <span  style="font-weight: bold;">534</span>: A69</font>    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958862&pid=S1409-2433201400020000200003&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[4] Bartelmann, M.; Schneider P. (2001) &#8220;Weak gravitational lensing&#8221;, <span style="font-style: italic;">Physics Reports</span> <span  style="font-weight: bold;">340</span>(4-5): 291&#8211;472.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958864&pid=S1409-2433201400020000200004&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[5] Binney, J.; Tremaine, S. (1987) <span style="font-style: italic;">Galactic Dynamics</span>. Princeton University Press, Princeton NJ.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958867&pid=S1409-2433201400020000200005&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[6] Cardone, V.F.; Piedipalumbo, E.; Tortora, C. (2005) &#8220;Spherical galaxy models with power-law logarithmic slope&#8221;, <span  style="font-style: italic;">MNRAS</span> <span  style="font-weight: bold;">358</span>: 1325&#8211;1336.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958870&pid=S1409-2433201400020000200006&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --> </font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[7] Chemin, L.; de Blok, W.J.G.; Mamon, G.A. (2011) &#8220;Improved modeling of the mass distribution of disk galaxies by the Einasto halo model&#8221;, <span style="font-style: italic;">ApJ</span> <span  style="font-weight: bold;">142</span>: 109&#8211;124.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958873&pid=S1409-2433201400020000200007&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --> </font>    ]]></body>
<body><![CDATA[<br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[8] de Blok,W. J. G. (2010) &#8220;The core-cusp problem&#8221;, <span style="font-style: italic;">Advances in Astronomy</span>, <span style="font-weight: bold;">2010</span>: 1&#8211;14.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958876&pid=S1409-2433201400020000200008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[9] Dhar, B.K.; Williams, L.L.R. (2011) &#8220;Surface brightness and intrinsic luminosity of ellipticals&#8221;, <span style="font-style: italic;">MNRAS</span>, <span style="font-weight: bold;">427</span>: 204&#8211;244.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958879&pid=S1409-2433201400020000200009&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[10] Dutton, A. and Maccio, A. (2014) &#8220;Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles&#8221;, to appear in <span style="font-style: italic;">MNRAS</span>, <span style="font-style: italic;">arXiv</span>:1402.7073.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958882&pid=S1409-2433201400020000200010&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     ]]></body>
<body><![CDATA[<!-- ref --><br> <font style="font-family: Verdana;" size="2">[11] Einasto, J. (1965) &#8220;On the construction of a composite model for the Galaxy and on the determination of the system of Galactic parameters&#8221;, Trudy Inst. Astroz. <span style="font-style: italic;">Alma-Ata</span> <span style="font-weight: bold;">17</span>(1): 87&#8211;100.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958885&pid=S1409-2433201400020000200011&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[12] Fikioris, G. (2007) &#8220;Mellin transformmethod for integral evaluation: introduction and applications to electromagnetics&#8221; <span style="font-style: italic;">Synthesis Lectures on Computational Electromagnetics</span> <span style="font-weight: bold;">2</span>(1): 1&#8211;67</font>    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958888&pid=S1409-2433201400020000200012&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[13] Fox, C. (1961) &#8220;The G and H functions as symmetrical Fourier kernels&#8221;, <span style="font-style: italic;">Transactions of the American Mathematical Society</span> <span style="font-weight: bold;">98</span>: 395&#8211;429.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958890&pid=S1409-2433201400020000200013&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[14] Marichev, O.I. (1982) <span style="font-style: italic;">Handbook of Integral Transforms of Higher Transcendental Functions: Theory and Algorithmic Tables.</span> Ellis Horwood, Chichester.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958893&pid=S1409-2433201400020000200014&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    ]]></body>
<body><![CDATA[<br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[15] Meijer, C. S. (1936) &#8220;Uber Whittakersche bezw. Besselsche Funktionen und deren Produkte&#8221;, <span style="font-style: italic;">Nieuw Archief voor Wiskunde</span> <span style="font-weight: bold;">18</span>: 10&#8211;39.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958896&pid=S1409-2433201400020000200015&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[16] Meneghetti, M. et al. (2014) &#8220;The MUSIC of CLASH: predictions on the concentration-mass relation&#8221;, arXiv:1404.1384.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958899&pid=S1409-2433201400020000200016&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[17] Narayan, R.; Bartelmann, M. (1995) &#8220;Lectures on gravitational lensing&#8221;, en: A. Dekel &amp; J. P. Ostriker (Eds.) <span  style="font-style: italic;">Formation of Structure in the Universe</span> (Proceedings of the 1995 JerusalemWinter School), Cambridge University Press, London.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958902&pid=S1409-2433201400020000200017&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     ]]></body>
<body><![CDATA[<!-- ref --><br> <font style="font-family: Verdana;" size="2">[18] Navarro, J.F.; Frenk, C.S.; White, S.D.M. (1996) &#8220;The structure of cold dark matter halos&#8221;, <span style="font-style: italic;">ApJ</span> <span  style="font-weight: bold;">462</span>: 563&#8211;575.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958905&pid=S1409-2433201400020000200018&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[19] Navarro, J.F.; Frenk, C.S.; White, S.D.M. (1997) &#8220;A universal density profile from hierarchical clustering&#8221;, <span  style="font-style: italic;">MNRAS</span> <span  style="font-weight: bold;">490</span>: 493&#8211;508.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958908&pid=S1409-2433201400020000200019&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[20] Navarro, J.F., et al. (2010) &#8220;The diversity and similarity of simulated cold dark matter haloes&#8221;, <span style="font-style: italic;">MNRAS</span> <span style="font-weight: bold;">402</span>: 21&#8211;34.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958911&pid=S1409-2433201400020000200020&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[21] Retana-Montenegro, E.; Van Hese, E.; Gentile, G.; Baes, M.; Frutos-Alfaro, F. (2012) &#8220;Analytical properties of Einasto dark matter haloes&#8221;, A &amp; A, <span style="font-weight: bold;">540</span>: A70 (10p). (arXiv:1202.5242).    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958914&pid=S1409-2433201400020000200021&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[22] Schneider, P.; Ehlers, J.; Falco, E. E. (1992) <span style="font-style: italic;">Gravitational Lenses</span>. Springer, Berlin.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958917&pid=S1409-2433201400020000200022&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[23] Spergel, D.N., et al. (2003) &#8220;First year Wilkinson microwave anisotropy probe (WMAP) observations: Determination of cosmological parameters&#8221;, <span style="font-style: italic;">Astrophys.J.Suppl.</span><span  style="font-weight: bold;">148</span>: 175&#8211;194.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958920&pid=S1409-2433201400020000200023&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    <br>     <!-- ref --><br> <font style="font-family: Verdana;" size="2">[24] Novak, G.S., et al. (2012) &#8220;On galaxies and homology&#8221;, <span style="font-style: italic;">MNRAS</span>, <span style="font-weight: bold;">424</span>: 635&#8211;648.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1958923&pid=S1409-2433201400020000200024&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font>    ]]></body>
<body><![CDATA[<br> </div>     <br> <font style="font-family: Verdana;" size="2"><a name="1"></a><a  href="#3">*</a> Escuela de F&iacute;sica, Universidad de Costa Rica, San Pedro 11501, Costa Rica. E-mail: edwin@</font><font style="font-family: Verdana;" size="2">fisica.ucr.ac.cr</font>    <br>     <br> <font style="font-family: Verdana;" size="2"><a name="2"></a><a  href="#4">&#8224;</a> Escuela de F&iacute;sica, Universidad de Costa Rica, San Pedro 11501, Costa Rica. E-mail: frutos@</font><font style="font-family: Verdana;" size="2">fisica.ucr.ac.cr</font>    <br> <hr style="width: 100%; height: 2px;">     <div style="text-align: center;"><font style="font-family: Verdana;"  size="2"><span style="font-weight: bold;">Received: 22/Feb/2012; Revised: 4/Jun/2014; Accepted: 5/Jun/2014</span></font></div> <font style="font-family: Verdana;" size="2"></font></div>      ]]></body><back>
<ref-list>
<ref id="B1">
<label>1</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Adamchick]]></surname>
<given-names><![CDATA[V.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Definite integration in Mathematica V3.0]]></article-title>
<source><![CDATA[Mathematica in Education and Research]]></source>
<year>1996</year>
<volume>5</volume>
<numero>16-22</numero>
<issue>16-22</issue>
</nlm-citation>
</ref>
<ref id="B2">
<label>2</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Baes]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[Gentile]]></surname>
<given-names><![CDATA[G.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Analytical expressions for the deprojected Sérsic model]]></article-title>
<source><![CDATA[A & A]]></source>
<year>2011</year>
<volume>525</volume>
<numero>A136+</numero>
<issue>A136+</issue>
<page-range>1-7</page-range></nlm-citation>
</ref>
<ref id="B3">
<label>3</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Baes]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[van Hese]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Analytical expressions for the deprojected Sérsic model II: General expressions in terms of the Fox H function]]></article-title>
<source><![CDATA[A & A]]></source>
<year>2011</year>
<volume>534</volume>
<numero>A69</numero>
<issue>A69</issue>
</nlm-citation>
</ref>
<ref id="B4">
<label>4</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Bartelmann]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[Schneider]]></surname>
<given-names><![CDATA[P.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Weak gravitational lensing]]></article-title>
<source><![CDATA[Physics Reports]]></source>
<year>2001</year>
<volume>340</volume>
<numero>4-5</numero>
<issue>4-5</issue>
<page-range>291-472</page-range></nlm-citation>
</ref>
<ref id="B5">
<label>5</label><nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Binney]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<name>
<surname><![CDATA[Tremaine]]></surname>
<given-names><![CDATA[S.]]></given-names>
</name>
</person-group>
<source><![CDATA[Galactic Dynamics]]></source>
<year>1987</year>
<publisher-loc><![CDATA[Princeton^eNJ NJ]]></publisher-loc>
<publisher-name><![CDATA[Princeton University Press]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B6">
<label>6</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Cardone]]></surname>
<given-names><![CDATA[V.F.]]></given-names>
</name>
<name>
<surname><![CDATA[Piedipalumbo]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
<name>
<surname><![CDATA[Tortora]]></surname>
<given-names><![CDATA[C.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Spherical galaxy models with power-law logarithmic slope]]></article-title>
<source><![CDATA[MNRAS]]></source>
<year>2005</year>
<volume>358</volume>
<page-range>1325-1336</page-range></nlm-citation>
</ref>
<ref id="B7">
<label>7</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Chemin]]></surname>
<given-names><![CDATA[L.]]></given-names>
</name>
<name>
<surname><![CDATA[de Blok]]></surname>
<given-names><![CDATA[W.J.G.]]></given-names>
</name>
<name>
<surname><![CDATA[Mamon]]></surname>
<given-names><![CDATA[G.A.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Improved modeling of the mass distribution of disk galaxies by the Einasto halo model]]></article-title>
<source><![CDATA[ApJ]]></source>
<year>2011</year>
<volume>142</volume>
<page-range>109-124</page-range></nlm-citation>
</ref>
<ref id="B8">
<label>8</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[de Blok]]></surname>
<given-names><![CDATA[W. J. G.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[The core-cusp problem]]></article-title>
<source><![CDATA[Advances in Astronomy]]></source>
<year>2010</year>
<volume>2010</volume>
<page-range>1-14</page-range></nlm-citation>
</ref>
<ref id="B9">
<label>9</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Dhar]]></surname>
<given-names><![CDATA[B.K.]]></given-names>
</name>
<name>
<surname><![CDATA[Williams]]></surname>
<given-names><![CDATA[L.L.R.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Surface brightness and intrinsic luminosity of ellipticals]]></article-title>
<source><![CDATA[MNRAS]]></source>
<year>2011</year>
</nlm-citation>
</ref>
<ref id="B10">
<label>10</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Dutton]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
<name>
<surname><![CDATA[Maccio]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles]]></article-title>
<source><![CDATA[MNRAS]]></source>
<year>2014</year>
</nlm-citation>
</ref>
<ref id="B11">
<label>11</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Einasto]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[On the construction of a composite model for the Galaxy and on the determination of the system of Galactic parameters]]></article-title>
<source><![CDATA[Trudy Inst]]></source>
<year>1965</year>
<volume>17</volume>
<numero>1</numero>
<issue>1</issue>
<page-range>87-100</page-range></nlm-citation>
</ref>
<ref id="B12">
<label>12</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Fikioris]]></surname>
<given-names><![CDATA[G.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Mellin transformmethod for integral evaluation: introduction and applications to electromagnetics]]></article-title>
<source><![CDATA[Synthesis Lectures on Computational Electromagnetics]]></source>
<year>2007</year>
<volume>2</volume><volume>1</volume>
<page-range>1-67</page-range></nlm-citation>
</ref>
<ref id="B13">
<label>13</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Fox]]></surname>
<given-names><![CDATA[C.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[The G and H functions as symmetrical Fourier kernels]]></article-title>
<source><![CDATA[Transactions of the American Mathematical Society]]></source>
<year>1961</year>
<volume>98</volume>
<page-range>395-429</page-range></nlm-citation>
</ref>
<ref id="B14">
<label>14</label><nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Marichev]]></surname>
<given-names><![CDATA[O.I.]]></given-names>
</name>
</person-group>
<source><![CDATA[Handbook of Integral Transforms of Higher Transcendental Functions: Theory and Algorithmic Tables]]></source>
<year>1982</year>
<publisher-loc><![CDATA[Chichester ]]></publisher-loc>
<publisher-name><![CDATA[Ellis Horwood]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B15">
<label>15</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Meijer]]></surname>
<given-names><![CDATA[C. S.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Uber Whittakersche bezw. Besselsche Funktionen und deren Produkte]]></article-title>
<source><![CDATA[Nieuw Archief voor Wiskunde]]></source>
<year>1936</year>
<volume>18</volume>
<page-range>10-39</page-range></nlm-citation>
</ref>
<ref id="B16">
<label>16</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Meneghetti]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[The MUSIC of CLASH: predictions on the concentration-mass relation]]></article-title>
<source><![CDATA[arXiv]]></source>
<year>2014</year>
</nlm-citation>
</ref>
<ref id="B17">
<label>17</label><nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Narayan]]></surname>
<given-names><![CDATA[R.]]></given-names>
</name>
<name>
<surname><![CDATA[Bartelmann]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Lectures on gravitational lensing]]></article-title>
<person-group person-group-type="editor">
<name>
<surname><![CDATA[Dekel]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
<name>
<surname><![CDATA[Ostriker]]></surname>
<given-names><![CDATA[J. P.]]></given-names>
</name>
</person-group>
<source><![CDATA[Formation of Structure in the Universe (Proceedings of the 1995 JerusalemWinter School)]]></source>
<year>1995</year>
<publisher-loc><![CDATA[London ]]></publisher-loc>
<publisher-name><![CDATA[Cambridge University Press]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B18">
<label>18</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Navarro]]></surname>
<given-names><![CDATA[J.F.]]></given-names>
</name>
<name>
<surname><![CDATA[C.S.]]></surname>
<given-names><![CDATA[Frenk]]></given-names>
</name>
<name>
<surname><![CDATA[S.D.M.]]></surname>
<given-names><![CDATA[White]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[The structure of cold dark matter halos]]></article-title>
<source><![CDATA[ApJ]]></source>
<year>1996</year>
<volume>462</volume>
<page-range>563-575</page-range></nlm-citation>
</ref>
<ref id="B19">
<label>19</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Navarro]]></surname>
<given-names><![CDATA[J.F.]]></given-names>
</name>
<name>
<surname><![CDATA[Frenk]]></surname>
<given-names><![CDATA[C.S.]]></given-names>
</name>
<name>
<surname><![CDATA[White]]></surname>
<given-names><![CDATA[S.D.M.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[A universal density profile from hierarchical clustering]]></article-title>
<source><![CDATA[MNRAS]]></source>
<year>1997</year>
<volume>490</volume>
<page-range>493-508</page-range></nlm-citation>
</ref>
<ref id="B20">
<label>20</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Navarro]]></surname>
<given-names><![CDATA[J.F.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[The diversity and similarity of simulated cold dark matter haloes]]></article-title>
<source><![CDATA[MNRAS]]></source>
<year>2010</year>
<volume>402</volume><volume>21-34</volume>
</nlm-citation>
</ref>
<ref id="B21">
<label>21</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Retana-Montenegro]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
<name>
<surname><![CDATA[Van Hese]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
<name>
<surname><![CDATA[Gentile]]></surname>
<given-names><![CDATA[G.]]></given-names>
</name>
<name>
<surname><![CDATA[Baes]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[Frutos-Alfaro]]></surname>
<given-names><![CDATA[F.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Analytical properties of Einasto dark matter haloes]]></article-title>
<source><![CDATA[A & A]]></source>
<year>2012</year>
<volume>540</volume>
<numero>A70</numero>
<issue>A70</issue>
<page-range>10</page-range></nlm-citation>
</ref>
<ref id="B22">
<label>22</label><nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Schneider]]></surname>
<given-names><![CDATA[P.]]></given-names>
</name>
<name>
<surname><![CDATA[Ehlers]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<name>
<surname><![CDATA[Falco]]></surname>
<given-names><![CDATA[E. E.]]></given-names>
</name>
</person-group>
<source><![CDATA[Gravitational Lenses]]></source>
<year>1992</year>
<publisher-loc><![CDATA[^eBerlin Berlin]]></publisher-loc>
<publisher-name><![CDATA[Springer]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B23">
<label>23</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Spergel]]></surname>
<given-names><![CDATA[D.N.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[First year Wilkinson microwave anisotropy probe (WMAP) observations: Determination of cosmological parameters]]></article-title>
<source><![CDATA[Astrophys.J.]]></source>
<year>2003</year>
<volume>148</volume>
<numero>^sSuppl</numero>
<issue>^sSuppl</issue>
<supplement>Suppl</supplement>
<page-range>175-194</page-range></nlm-citation>
</ref>
<ref id="B24">
<label>24</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Novak]]></surname>
<given-names><![CDATA[G.S.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[On galaxies and homology]]></article-title>
<source><![CDATA[MNRAS]]></source>
<year>2012</year>
<volume>424</volume>
<page-range>635-648</page-range></nlm-citation>
</ref>
</ref-list>
</back>
</article>
